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Chemical Pressure Effects on the Stokes Shift of Bi3+ Luminescence in Orthorhombic Perovskites

  • A. M. Srivastava*
  • , M. G. Brik
  • , W. W. Beers
  • , W. Cohen
  • *Šī darba korespondējošais autors
  • Current Chemicals
  • Chongqing University of Posts and Telecommunications
  • University of Tartu
  • Jan Dlugosz University in Czestochowa
  • Academy of Romanian Scientists
  • University of Belgrade

Zinātniskās darbības rezultāts: Devums žurnālamZinātniskais raksts (žurnālā)koleģiāli recenzēts

5 Atsauces (Scopus)

Kopsavilkums

The relationship between the Stokes shift of Bi3+ emission and the volume of the unit-cell in two series of orthorhombic perovskites, LnB3+O3 (Ln = La, Gd, Y; B3+ = Al, In, Ga) and AB4+O3 (A = Ca, Sr; B4+ = Zr, Sn) is explored. The Stokes shift increases linearly with increasing cell volume. This is explained qualitatively by the lattice chemical pressure acting on the Bi3+ ion. The degree of Bi3+ ion off-centering displacement, which is due to the stereochemical activity of the lone-pair electrons (6s2), is controlled by the chemical pressure. A small cell suppresses the off-centering displacement to produce a small Stokes shift of emission by limiting the excited state structural distortion. In large cell, the off-centering displacement is more easily accommodated. The elimination of ground state distortion in the excited state gives larger Stokes shift of emission. These qualitative arguments are supplemented by recent first-principles calculations on Bi3+ luminescence in these perovskites. The Bi3+ luminescence in SrZrO3, previously assigned to emission from the D-state, is now assigned to the localized 3P0,11S0 transition. The energy of the 1S03P1 transition is correlated with the covalence of the BO6/2 perovskite framework. Discussion on the effective ionic radius of the Bi3+ ion in these perovskites is presented.

OriģinālvalodaAngļu
Raksta numurs096003
ŽurnālsECS Journal of Solid State Science and Technology
Sējums11
Izdevuma numurs9
DOIs
Publikācijas statussPublicēts - sept. 2022
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